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Primordial Black Holes as a dark matter candidate (2020)
Journal Article
Green, A. M., & Kavanagh, B. J. (2021). Primordial Black Holes as a dark matter candidate. Journal of Physics G: Nuclear and Particle Physics, 48(4), Article 043001. https://doi.org/10.1088/1361-6471/abc534

The detection of gravitational waves from mergers of tens of Solar mass black hole binaries has led to a surge in interest in Primordial Black Holes (PBHs) as a dark matter candidate. We aim to provide a (relatively) concise overview of the status of... Read More about Primordial Black Holes as a dark matter candidate.

Constraints on the cosmic string loop collapse fraction from primordial black holes (2020)
Journal Article
James-Turner, C., Weil, D. P. B., Green, A. M., & Copeland, E. J. (2020). Constraints on the cosmic string loop collapse fraction from primordial black holes. Physical Review D, 101(12), Article 123526. https://doi.org/10.1103/physrevd.101.123526

A small fraction, f , of cosmic string loops can collapse to form Primordial Black Holes (PBHs). Constraints on the abundance of PBHs can therefore be used to constrain f. We update these calculations, taking into account the PBH extended mass functi... Read More about Constraints on the cosmic string loop collapse fraction from primordial black holes.

Understanding the suppression of structure formation from dark matter-dark energy momentum coupling (2020)
Journal Article
Chamings, F. N., Avgoustidis, A., Copeland, E. J., Green, A. M., & Pourtsidou, A. (2020). Understanding the suppression of structure formation from dark matter-dark energy momentum coupling. Physical Review D, 101(4), https://doi.org/10.1103/physrevd.101.043531

Models in which scalar field dark energy interacts with dark matter via a pure momentum coupling have previously been found to potentially ease the structure formation tension between early-and late-universe observations. In this article we explore t... Read More about Understanding the suppression of structure formation from dark matter-dark energy momentum coupling.

Early dark energy constraints on growing neutrino quintessence cosmologies (2019)
Journal Article
Noble Chamings, F., Avgoustidis, A., Copeland, E. J., Green, A. M., & Li, B. (2019). Early dark energy constraints on growing neutrino quintessence cosmologies. Physical Review D, 100(4), https://doi.org/10.1103/physrevd.100.043525

We investigate cosmological models in which dynamical dark energy consists of a scalar field whose present-day value is controlled by a coupling to the neutrino sector. The behavior of the scalar field depends on three functions: a kinetic function,... Read More about Early dark energy constraints on growing neutrino quintessence cosmologies.

Pitfalls of a power-law parametrization of the primordial power spectrum for primordial black hole formation (2018)
Journal Article
Green, A. M. (2018). Pitfalls of a power-law parametrization of the primordial power spectrum for primordial black hole formation. Physical Review D, 98(2), https://doi.org/10.1103/PhysRevD.98.023529

Primordial Black Holes (PBHs) can form in the radiation dominated early Universe from the collapse of large density perturbations produced by inflation. A power-law parameterisation of the primordial power spectrum is often used to extrapolate from c... Read More about Pitfalls of a power-law parametrization of the primordial power spectrum for primordial black hole formation.

Astrophysical uncertainties on stellar microlensing constraints on multi-solar mass primordial black hole dark matter (2017)
Journal Article
Green, A. M. (2017). Astrophysical uncertainties on stellar microlensing constraints on multi-solar mass primordial black hole dark matter. Physical Review D, 96, Article 043020. https://doi.org/10.1103/PhysRevD.96.043020

There has recently been interest in multi-Solar mass Primordial Black Holes (PBHs) as a dark matter (DM) candidate. There are various microlensing, dynamical and accretion constraints on the abundance of PBHs in this mass range. Taken at face value t... Read More about Astrophysical uncertainties on stellar microlensing constraints on multi-solar mass primordial black hole dark matter.

Astrophysical uncertainties on the local dark matter distribution and direct detection experiments (2017)
Journal Article
Green, A. M. (2017). Astrophysical uncertainties on the local dark matter distribution and direct detection experiments. Journal of Physics G: Nuclear and Particle Physics, 44(8), https://doi.org/10.1088/1361-6471/aa7819

The differential event rate in weakly interacting massive particle (WIMP) direct detection experiments depends on the local dark matter density and velocity distribution. Accurate modelling of the local dark matter distribution is therefore required... Read More about Astrophysical uncertainties on the local dark matter distribution and direct detection experiments.

Microlensing and dynamical constraints on primordial black hole dark matter with an extended mass function (2016)
Journal Article
Green, A. M. (in press). Microlensing and dynamical constraints on primordial black hole dark matter with an extended mass function. Physical Review D - Particles, Fields, Gravitation and Cosmology, 94, Article 063530. https://doi.org/10.1103/PhysRevD.94.063530

The recent discovery of gravitational waves from mergers of ∼10 M⊙ black hole binaries has stimulated interested in primordial black hole (PBH) dark matter in this mass range. Microlensing and dynamical constraints exclude all of the dark matter in c... Read More about Microlensing and dynamical constraints on primordial black hole dark matter with an extended mass function.

How to calculate dark matter direct detection exclusion limits that are consistent with gamma rays from annihilation in the Milky Way halo (2016)
Journal Article
Cerdeno, D. G., Fornasa, M., Green, A. M., & Peiro, M. (2016). How to calculate dark matter direct detection exclusion limits that are consistent with gamma rays from annihilation in the Milky Way halo. Physical Review D, 94, Article 043516. https://doi.org/10.1103/PhysRevD.94.043516

When comparing constraints on the weakly interacting massive particle (WIMP) properties from direct and indirect detection experiments it is crucial that the assumptions made about the dark matter (DM) distribution are realistic and consistent. For i... Read More about How to calculate dark matter direct detection exclusion limits that are consistent with gamma rays from annihilation in the Milky Way halo.

A review of the discovery reach of directional Dark Matter detection (2016)
Journal Article
Mayet, F., Green, A. M., Battat, J., Billard, J., Bozorgnia, N., Gelmini, G., …Vahsen, S. (2016). A review of the discovery reach of directional Dark Matter detection. Physics Reports, 627, https://doi.org/10.1016/j.physrep.2016.02.007

Cosmological observations indicate that most of the matter in the Universe is Dark Matter. Dark Matter in the form of Weakly Interacting Massive Particles (WIMPs) can be detected directly, via its elastic scattering off target nuclei. Most current di... Read More about A review of the discovery reach of directional Dark Matter detection.

WIMP particle physics and astrophysics with direct detection and neutrino telescope data (2015)
Journal Article
Kavanagh, B. J., Fornasa, M., & Green, A. M. (2015). WIMP particle physics and astrophysics with direct detection and neutrino telescope data. Physical Review D - Particles, Fields, Gravitation and Cosmology, 91, Article 103533

With positive signals from multiple direct detection experiments it will, in principle, be possi- ble to measure the mass and cross sections of weakly-interacting massive particle (WIMP) dark matter. Recent work has shown that, with a polynomial para... Read More about WIMP particle physics and astrophysics with direct detection and neutrino telescope data.

WIMP physics with ensembles of direct-detection experiments (2014)
Journal Article
Peter, A. H., Glusevic, V., Green, A. M., Kavanagh, B. J., & Lee, S. L. (2014). WIMP physics with ensembles of direct-detection experiments. Physics of the Dark Universe, 5-6, https://doi.org/10.1016/j.dark.2014.10.006

The search for weakly-interacting massive particle (WIMP) dark matter is multi-pronged. Ulti- mately, the WIMP-dark-matter picture will only be confirmed if different classes of experiments see consistent signals and infer the same WIMP properties. I... Read More about WIMP physics with ensembles of direct-detection experiments.

Self-consistent phase-space distribution function for the anisotropic dark matter halo of the Milky Way (2014)
Journal Article
Fornasa, M., & Green, A. M. (2014). Self-consistent phase-space distribution function for the anisotropic dark matter halo of the Milky Way. Physical Review D - Particles, Fields, Gravitation and Cosmology, 89(6), Article 063531. https://doi.org/10.1103/physrevd.89.063531

Dark Matter (DM) direct detection experiments usually assume the simplest possible ‘Standard Halo Model’ for the Milky Way (MW) halo in which the velocity distribution is Maxwellian. This model assumes that the MW halo is an isotropic, isothermal sph... Read More about Self-consistent phase-space distribution function for the anisotropic dark matter halo of the Milky Way.